The Metropolis-Hastings simulation algorithm
rmh
is run for
nrep[1]
steps at inverse temperature invtemp[1]
,
then for
nrep[2]
steps at inverse temperature invtemp[2]
,
and so on.
Setting the inverse temperature to a value \(\alpha\)
means that the probability density of the Gibbs model, \(f(x)\),
is replaced by \(g(x) = C\, f(x)^\alpha\)
where \(C\) is a normalising constant depending on
\(\alpha\).
Larger values of \(\alpha\) exaggerate the high and low
values of probability density, while smaller values of \(\alpha\)
flatten out the probability density.
For example if the original model
is a Strauss process,
the modified model is close to a hard core process
for large values of inverse temperature, and close to a Poisson process
for small values of inverse temperature.